|- Apache Point
|- 2.5-m Telescope
|Details of the Data
Before astronomers can make a map of the sky, they need a telescope. Past surveys,
such as the Palomar Sky Survey, were done with Schmidt telescopes with correcting
lenses 48 inches (1.5 m) across. To map more distant, fainter objects, Sloan
astronomers decided to build a brand new telescope with lenses 2.5 meters (100 inches)
Apache Point Observatory
The SDSS telescopes are located at
Apache Point Observatory (APO)
in Sunspot, New Mexico. The observatory is surrounded by the Lincoln National
Forest in the Sacramento Mountains, and sits on a mountain 9,200 feet above sea level,
where the atmosphere contains little water vapor and few pollutants. Because the site
is so high and so far from major cities, the night sky seen from APO is among the
darkest in the United States.
In addition to the SDSS telescopes, the APO also houses a 3.5-meter telescope and
New Mexico State University's 1.0-meter telescope.
The Main 2.5-meter Telescope
Because the SDSS telescope will make
a map of the whole sky, it must produce in-focus images over a large field of view.
Most modern telescopes, like the huge 10-meter
Keck telescopes in
Hawaii, are used to observe small patches of sky at a time. To see a large area of sky
at once, the SDSS telescope required a different and complex design.
The inside of the telescope is
dominated by two reflecting mirrors. Light reflects from the mirrors into a focusing
system that includes two corrective lenses, which minimize distortion. The diagram
at right shows how that incoming starlight strikes the 2.5-meter primary mirror,
bounces back and strikes the smaller (1.08-meter) secondary mirror, then is
reflected back through a hole in the primary mirror. The light passes through
the first correcting lens and then through the second lens on top of the camera.
The telescope can take sharply focused images from an area of three degrees,
equal to the diameter of about 30 full moons.
Although this design looks like a typical Cassegrain telescope, the mirror
surfaces are of a different shape, and the focusing system uses an additional
corrective element. The telescope's housing is also unique. Most telescopes
are kept inside domes, with only a small slit in the dome for observing.
However, this arrangement often causes heat become trapped inside the dome during
the day. When the heat is released at night, the escaping heat causes air turbulence
that blurs the telescope's images. To avoid this problem, the SDSS telescope is
completely removed from its enclosure, and carries its own wind baffle
(the metallic box around the telescope tube).
The Photometric Telescope
In addition to the main telescope, the SDSS uses this 0.5-meter Photometric Telescope to monitor subtle changes in the atmospheric temperature and pressure during the course of the survey. This information allows astronomers to calibrate an object's brightness as measured with the main telescope.